Mon. Not. R. Astron. Soc., 466, 2261-2271 (2017/April-1)
System mass constraints for the accreting millisecond pulsar XTE J1814-338 using Bowen fluorescence.
WANG L., STEEGHS D., CASARES J., CHARLES P.A., MUNOZ-DARIAS T., MARSH T.R., HYNES R.I. and O'BRIEN K.
Abstract (from CDS):
We present phase-resolved spectroscopy of the millisecond X-ray pulsar XTE J1814-338 obtained during its 2003 outburst. The spectra are dominated by high-excitation emission lines of He II λ4686, Hβ, and the Bowen blend C III/N III 4630-50 Å. We exploit the proven Bowen fluorescence technique to establish a complete set of dynamical system parameter constraints using bootstrap Doppler tomography, a first for an accreting millisecond X-ray pulsar binary. The reconstructed Doppler map of the N III λ4640 Bowen transition exhibits a statistically significant (>4σ) spot feature at the expected position of the companion star. If this feature is driven by irradiation of the surface of the Roche lobe filling companion, we derive a strict lower limit to the true radial velocity semi-amplitude K2. Combining our donor constraint with the well-constrained orbit of the neutron star leads to a determination of the binary mass ratio: q = 0.123+0.012–0.010. The component masses are not tightly constrained given our lack of knowledge of the binary inclination. We cannot rule out a canonical neutron star mass of 1.4 M☉ (1.1 M☉ < M1 < 3.1 M☉; 95 per cent). The 68/95 per cent confidence limits of M2 are consistent with the companion being a significantly bloated, M-type main-sequence star. Our findings, combined with results from studies of the quiescent optical counterpart of XTE J1814-338, suggest the presence of a rotation-powered millisecond pulsar in XTE J1814-338 during an X-ray quiescent state. The companion mass is typical of the so-called redback pulsar binary systems (M2 ∼ 0.2 M☉).
© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
accretion, accretion discs - binaries: close - stars: individual: XTE J1814-338 - X-rays: stars - X-rays: stars
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